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Cited by 874

The DOI matches its Crossref record; 25 of the 25 references it cites were found in a registry or an index.

Reconstruction of a Scalar-Tensor Theory of Gravity in an Accelerating Universe

Open access
Boisseau, B., Esposito-Farèse, G., Polarski, D., Starobinsky, A. A.·2000·Physical Review Letters

Abstract

The present acceleration of the Universe strongly indicated by recent observational data can be modeled in the scope of a scalar-tensor theory of gravity. We show that it is possible to determine the structure of this theory along with the present density of dustlike matter from two observable cosmological functions: the luminosity distance and the linear density perturbation in the dustlike matter component as functions of redshift. Explicit results are presented in the first order in the small inverse Brans-Dicke parameter omega(-1).

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Crossref · 10.1103/physrevlett.85.2236

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Metadata

Authors
Boisseau, B., Esposito-Farèse, G., Polarski, D., & Starobinsky, A. A.
Venue
Physical Review Letters
Published
2000-09-11
Volume
85
Issue
11
Pages
2236-2239
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2156404110
Cited by
874
References
25
FWCI
12.35
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Reconstruction of a Scalar-Tensor Theory of Gravity in an Accelerating Universe. https://app.cochat.ai/papers/10.1103/physrevlett.85.2236
The paper
Boisseau, B., Esposito-Farèse, G., Polarski, D., & Starobinsky, A. A. (2000). Reconstruction of a Scalar-Tensor Theory of Gravity in an Accelerating Universe. Physical Review Letters. https://doi.org/10.1103/physrevlett.85.2236

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.